A worldwide theoretical and experimental effort to search for dibaryons has lasted a long time. Although the research on the dibaryon has experienced several ups and downs in its history, dibaryons have received renewed interest in recent years. The well-known dibaryon resonance \(d^{*}\)  was repeatedly observed by the WASA detector at COSY [1]}, [2]}, [3]}, [4]}, [5]}, and extensively investigated within various theoretical approaches [6]}, [7]}, [8]}, [9]}, [10]}, [11]}, [12]}, [13]}.
Another dibaryon \(N\Omega \)  was proposed as a narrow resonance in a relativistic quark model [14]}, and was investigated by other quark models [15]}, [16]}, [17]}, [18]}, [19]}, [20]}, as well as the lattice QCD [21]}, [22]}. The progress of the \(N\Omega \)  searches by the STAR experiment at the Relativistic Heavy-Ion Collider (RHIC) favored the existence of \(N\Omega \)  [23]}. Besides, the study of the strong interaction among hadrons at the LHC by ALICE Collaboration also supported the possibility of forming the \(N\Omega \)  state [24]}.
